As can be seen from Eq. (REF ), the spherical black hole possesses an angular defect. Therefore, the thermodynamical quantities asociated to this configuation
must be calculated using the extended thermodynamic formalism [1]}, [2]}. Here we will follow the computations performed in Ref. [3]},
where the authors have studied the thermodynamics of the black hole in Ref. [4]}, which correponds to the \(SU(2)\) 
case of the spherical black hole constructed here,
but including the Skyrme termIn fact, one can compute the mass, temperature and entropy of our spherical black hole
simply rescaling, \(K \rightarrow a_N K\) , and doing, \(\lambda \rightarrow 0\) , in Ref. [3]}. (see also [6]}).
